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| HSCS J142903-010443 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST12:39:07 |
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trying to find the most relevant references on this object.
More on score
| Bibcode/DOI | Score |
in Title|Abstract| Keywords |
in a table | in teXt, Caption, ... | Nb occurence | Nb objects in ref |
Citations (from ADS) |
Title | First 3 Authors |
|---|---|---|---|---|---|---|---|---|---|
| 2017ApJ...849...91M | 21 | D | 1 | 22 | 227 | Physical properties of 15 quasars at z >= 6.5. | MAZZUCCHELLI C., BANADOS E., VENEMANS B.P., et al. | ||
| 2018PASJ...70S..35M | 17 | D | 1 | 66 | 104 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs). II. Discovery of 32 quasars and luminous galaxies at 5.7 < z ≤ 6.8. | MATSUOKA Y., ONOUE M., KASHIKAWA N., et al. | ||
2019MNRAS.490.2542P 
|
16 | D | 1 | 2245 | ~ | Unveiling the weak radio quasar population at z≥4. | PERGER K., FREY S., GABANYI K.E., et al. | ||
|
2020MNRAS.494..789R
|
16 | D | 1 | 489 | 25 | The near and mid-infrared photometric properties of known redshift z >= 5 quasars. | ROSS N.P. and CROSS N.J.G. | ||
|
2021A&A...656A.137G
|
17 | D | 1 | 493 | 12 | Low frequency radio properties of the z > 5 quasar population. | GLOUDEMANS A.J., DUNCAN K.J., ROTTGERING H.J.A., et al. | ||
|
2022ApJS..259...20H
|
17 | D | 1 | 1042 | 83 | GOLDRUSH. IV. Luminosity Functions and Clustering Revealed with ∼4,000,000 Galaxies at z ∼ 2-7: Galaxy-AGN Transition, Star Formation Efficiency, and Implication for Evolution at z > 10. | HARIKANE Y., ONO Y., OUCHI M., et al. | ||
| 2022MNRAS.517.1264L | 102 | D | F | 2 | 94 | 3 | Subaru High-z Exploration of Low-Luminosity Quasars (SHELLQs) - XV. Constraining the cosmic reionization at 5.5 < z < 7. | LU T.-Y., GOTO T., HASHIMOTO T., et al. | |
| 2023ApJ...949L..42M | 17 | D | 1 | 35 | 5 | Quasar Luminosity Function at z = 7. | MATSUOKA Y., ONOUE M., IWASAWA K., et al. | ||
| 2025MNRAS.540.1308O | 19 | D | 1 | 72 | ~ | Optical and near-infrared spectroscopy of quasars at z > 6.5: public data release and composite spectrum. | ONORATO S., HENNAWI J.F., SCHINDLER J.-T., et al. |
